5 Presentation of standard photometry data

Not all our nights were of photometric quality. The results presented in Table 4 only concern those observations that were acquired in "reasonable" or good photometric conditions. This comprises standard V magnitudes and (V-I) colour indices for the components of 203 Hipparcos double stars, one apparently double (the triple system ADS 6223) and 9 astrometric standard stars. Also presented are the magnitude differences, $\Delta\,V$ and $\Delta\,(V-I)$, between the components A and B of each system in the Cousins standard system. The first columns list the identifier (same as before), the Julian date, and the previously cited data along with standard deviations on all parameters. In the case that only one colour was obtained, one must note that the listed component magnitudes and differences, $\Delta\,V$ or $\Delta$i, are less accurate: in that case a default value of 0.7 for $(V-I)_{\rm A}$ and $(V-I)_{\rm B}$ was adopted in the reduction (as done in the standard Hipparcos double star processing). Such data are e.g. presented separately in Table 5 (filter I only). These results will be discussed and illustrated in Sect. 6.4.

 

 

Table 4: CCD VI photometry for 203 Hipparcos and 9 astrometric standard double stars.

Identifier	Jul. Dat.	nV	$V_{\rm A}$	$\sigma_{V_{\rm A}}$	$V_{\rm B}$	$\sigma_{V_{\rm B}}$	nI	$(V-I)_{\rm A}$	$\sigma_{(V-I)_{\rm A}}$	$(V-I)_{\rm B}$	$\sigma_{(V-I)_{\rm B}}$	$\Delta V$	$\Delta$(V-I)
	2440000+		(mag)	(mag)	(mag)	(mag)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
000045	8852.8460	7	9.755	.020	11.791	.022	7	.78	.03	1.32	.03	2.036	.55
000169	8851.8217	3	9.523	.020	10.885	.020	3	1.62	.03	1.96	.03	1.362	.34
000924	8849.8117	6	9.349	.060	11.150	.060	0	-	-	-	-	1.801	-
000924	8850.8464	6	9.155	.020	11.063	.020	7	.79	.03	1.29	.03	1.907	.50
001186	8852.8973	3	10.190	.021	11.351	.025	1	.68	.03	.75	.03	1.162	.07
002438	8852.9290	5	10.247	.020	13.225	.020	14	.56	.03	1.13	.03	2.978	.57
002438	9668.5774	2	10.244	.025	13.188	.025	0	-	-	-	-	2.944	-
002449	9668.5911	2	10.362	.051	10.839	.051	2	.72	.05	.63	.05	.477	-.09
002663	9670.5833	10	6.655	.025	8.590	.025	10	.65	.04	.92	.04	1.935	.27
003200	8851.8605	4	10.076	.020	11.357	.020	4	.63	.03	.73	.03	1.280	.10
003205	8851.8674	3	10.011	.020	10.223	.020	1	.52	.03	.46	.03	.212	-.06
003397	8848.8919	11	6.970	.030	10.573	.031	12	.51	.04	.18	.05	3.603	-.34
003827	8850.8527	2	9.640	.020	10.052	.020	3	.65	.03	.68	.03	.412	.03
004404	8850.8689	13	9.057	.020	12.388	.022	14	.59	.03	1.12	.03	3.332	.53
004764	9346.4528	6	9.698	.044	11.043	.134	3	.82	.06	1.04	.18	1.344	.23
005413	9346.4701	13	9.401	.020	11.657	.020	13	.22	.03	.97	.03	2.256	.75
005992	9670.6241	6	6.461	.025	8.314	.026	7	.02	.04	.46	.04	1.853	.44
006132	8851.8921	11	10.316	.020	12.270	.020	12	.69	.03	.89	.03	1.954	.20
006707	8941.6132	11	8.380	.019	9.762	.019	9	.44	.02	.56	.02	1.382	.12
007290	8851.9007	7	9.918	.020	12.998	.025	4	1.12	.03	2.52	.03	3.081	1.40
008054	8939.6481	7	9.902	.036	11.363	.036	4	.71	.04	.87	.04	1.461	.15
008236	8850.8941	4	9.952	.020	12.743	.020	4	.63	.03	1.00	.03	2.792	.37
008957	9347.4322	3	7.157	.017	7.249	.017	3	.35	.02	.40	.02	.093	.05
008965	9347.4362	3	8.825	.025	10.693	.100	3	.05	.04	.59	.17	1.868	.54
009258	9670.6556	6	7.194	.025	7.628	.026	2	.47	.04	.64	.04	.434	.17
009344	8850.9127	3	9.779	.020	9.987	.020	3	.53	.03	.55	.03	.208	.02
009651	8850.9180	3	9.960	.020	10.181	.020	3	.66	.03	.73	.03	.221	.07
010579	9668.6298	5	9.432	.020	9.905	.020	4	.64	.03	.73	.03	.473	.09
010683	8939.6568	4	8.130	.020	8.943	.020	3	.57	.03	.61	.03	.813	.04
010722	9347.4501	7	8.395	.025	10.518	.129	6	1.02	.03	.32	.17	2.123	-.70
010983	9669.6681	14	7.503	.026	10.669	.043	18	1.01	.04	.55	.06	3.166	-.45
011219	9668.7130	10	8.864	.020	10.129	.020	0	-	-	-	-	1.265	-
011257	9668.6486	4	9.124	.020	9.357	.020	5	.57	.03	.58	.03	.233	.02
011945	9348.4323	3	7.877	.017	7.980	.017	3	1.07	.02	1.05	.02	.103	-.02
012105	9668.7052	6	7.055	.021	8.922	.021	4	.95	.03	.24	.03	1.867	-.72
012708	9347.4560	3	6.998	.020	7.270	.021	5	-.09	.03	-.04	.03	.272	.04
012752	8939.7298	4	9.781	.024	10.891	.031	8	.75	.03	.80	.04	1.110	.05
013199	9348.4429	6	9.470	.017	9.831	.017	3	.52	.02	.47	.02	.361	-.05
013243	9345.4744	5	9.653	.021	9.773	.021	6	.78	.03	.84	.03	.120	.06
013815	9347.4836	13	8.250	.019	10.645	.073	14	-.03	.03	-.01	.09	2.395	.03
013866	9668.6967	6	10.013	.020	11.689	.020	4	.52	.03	.72	.03	1.676	.20
014584	9346.4783	12	9.553	.020	10.659	.020	2	.92	.03	.90	.03	1.106	-.02
015257	9349.4358	11	8.433	.018	10.689	.048	12	1.03	.03	1.09	.17	2.256	.06
015356	9346.5003	11	9.029	.020	11.205	.021	11	.40	.03	.54	.03	2.176	.14
015869	9348.4497	15	7.070	.017	8.963	.022	15	.18	.02	.23	.03	1.893	.05
015883	9347.4997	5	7.308	.018	8.848	.024	5	.25	.02	.62	.03	1.540	.36
016080	8941.7033	7	8.091	.019	9.853	.019	5	.53	.03	.79	.03	1.762	.26
017260	9347.5039	6	7.925	.026	8.871	.047	5	.30	.04	.69	.07	.946	.39
017288	9670.7485	5	7.815	.025	10.377	.030	0	-	-	-	-	2.562	-
017328	9349.4562	4	6.662	.017	8.042	.021	4	-.03	.02	.18	.03	1.381	.21

 

Table 4: continued.

Identifier	Jul. Dat.	nV	$V_{\rm A}$	$\sigma_{V_{\rm A}}$	$V_{\rm B}$	$\sigma_{V_{\rm B}}$	nI	$(V-I)_{\rm A}$	$\sigma_{(V-I)_{\rm A}}$	$(V-I)_{\rm B}$	$\sigma_{(V-I)_{\rm B}}$	$\Delta V$	$\Delta$(V-I)
	2440000+		(mag)	(mag)	(mag)	(mag)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
017397	8941.7226	13	9.532	.021	12.091	.021	23	.24	.03	.57	.03	2.559	.33
017436	9348.4574	11	6.549	.017	9.527	.019	0	-	-	-	-	2.978	-
017464	9349.4610	10	6.373	.017	9.465	.017	0	-	-	-	-	3.092	-
018068	9346.5063	7	8.000	.020	9.987	.021	0	-	-	-	-	1.987	-
018429	9345.5112	3	10.431	.021	10.495	.021	3	1.04	.03	1.07	.03	.063	.03
018883	9349.4728	3	8.321	.017	8.666	.017	3	.56	.02	.42	.02	.345	-.14
019684	9345.5212	3	8.194	.021	8.275	.021	0	-	-	-	-	.081	-
019892	9668.7629	10	7.387	.020	9.181	.020	5	-.01	.03	.52	.03	1.795	.52
019951	9345.5550	3	9.616	.020	10.014	.020	6	.77	.03	.66	.03	.397	-.12
020020	9347.5166	8	5.987	.018	7.685	.019	7	-.26	.02	-.12	.03	1.698	.15
020020	9669.7071	10	6.085	.029	7.808	.029	6	-.13	.04	.07	.04	1.723	.20
020374	9348.5275	8	7.657	.017	10.698	.043	9	1.09	.02	.89	.09	3.042	-.20
020735	9348.5139	4	7.053	.018	8.216	.021	7	-.02	.02	.23	.03	1.163	.24
020766	9349.4779	10	7.844	.017	10.322	.039	11	1.04	.03	.66	.10	2.478	-.37
020943	8940.7505	11	10.255	.050	12.218	.051	0	-	-	-	-	1.963	-
020956	8939.7424	10	10.363	.022	12.254	.023	0	-	-	-	-	1.891	-
021213	9348.5338	4	7.848	.017	9.615	.018	5	.18	.02	.45	.03	1.767	.27
021577	9348.4838	4	7.181	.017	9.047	.018	7	.33	.02	.49	.03	1.866	.16
021849	9348.5500	11	7.474	.017	9.976	.018	11	.22	.02	.61	.02	2.502	.39
022249	9349.4970	10	7.328	.017	9.990	.021	10	.53	.02	1.10	.03	2.662	.57
022463	8941.7542	3	8.958	.015	9.763	.016	2	.51	.02	.64	.02	.805	.13
022874	8940.7584	3	10.039	.053	10.312	.053	3	.53	.07	.57	.07	.273	.04
023196	9670.7778	5	7.194	.027	9.026	.027	7	.43	.04	.60	.04	1.832	.17
023480	8941.7664	5	8.008	.018	9.457	.040	5	.26	.02	.26	.04	1.449	-.01
023493	9668.8104	1	7.094	.020	8.629	.020	7	-.11	.03	.17	.03	1.535	.28
023644	9349.5198	3	8.912	.017	9.472	.018	3	.70	.03	.96	.03	.560	.27
024039	8939.7794	18	9.525	.021	14.402	.031	17	.78	.03	2.20	.04	4.877	1.42
024203	9669.7795	7	6.245	.029	7.446	.029	9	1.00	.04	.11	.04	1.201	-.89
024366	8941.7834	11	9.369	.015	11.081	.016	7	.73	.02	.73	.02	1.712	.00
024429	9349.5306	6	10.112	.018	10.070	.018	3	.60	.03	.39	.03	-.042	-.21
024717	9346.5535	8	9.171	.020	10.916	.025	8	.94	.03	.71	.04	1.746	-.23
025231	9349.5469	7	7.896	.021	9.460	.051	8	.49	.04	1.25	.09	1.564	.76
025482	9349.5348	4	6.565	.018	7.120	.019	3	.24	.03	.74	.03	.555	.50
026401	8941.7900	5	9.650	.017	10.538	.017	5	.75	.02	.93	.02	.888	.18
027174	9349.5682	5	8.558	.017	10.234	.024	6	.53	.02	.87	.03	1.676	.34
027386	9670.8134	3	6.059	.028	6.095	.028	4	.38	.05	.26	.05	.036	-.13
027424	8940.7983	2	9.163	.051	9.306	.051	4	-.14	.08	-.09	.08	.143	.05
027427	9669.7865	12	7.311	.026	9.912	.026	11	-.08	.04	.48	.04	2.601	.56
027524	9346.5577	4	9.364	.020	9.745	.020	4	.75	.03	.71	.03	.382	-.04
027526	9346.5772	4	10.803	.020	10.997	.020	4	.53	.03	.88	.03	.194	.35
027827	9349.5637	4	8.612	.019	9.864	.031	4	-.01	.03	.40	.04	1.252	.41
027922	9347.5607	9	7.542	.017	10.648	.017	9	.76	.02	1.66	.02	3.106	.90
027962	9670.8204	13	6.906	.027	9.178	.027	13	-.06	.04	.39	.04	2.272	.45
028165	9349.5824	3	8.351	.018	8.857	.019	6	.29	.03	.54	.03	.506	.25
028275	9347.5670	3	8.625	.017	8.746	.017	3	.33	.02	.37	.02	.121	.04
028383	9346.5898	4	9.516	.021	10.506	.024	4	.36	.04	1.84	.05	.990	1.48
028819	9346.5943	5	9.722	.021	11.362	.039	5	.83	.03	1.03	.06	1.640	.19
028852	9348.5975	4	8.257	.017	8.465	.017	3	.44	.02	.46	.02	.208	.02
029622	8939.8235	1	9.197	.020	10.326	.020	2	.73	.03	.70	.03	1.129	-.03
029811	9347.5776	5	7.069	.018	8.383	.028	5	.50	.03	.40	.04	1.314	-.09

 

Table 4: continued.

Identifier	Jul. Dat.	nV	$V_{\rm A}$	$\sigma_{V_{\rm A}}$	$V_{\rm B}$	$\sigma_{V_{\rm B}}$	nI	$(V-I)_{\rm A}$	$\sigma_{(V-I)_{\rm A}}$	$(V-I)_{\rm B}$	$\sigma_{(V-I)_{\rm B}}$	$\Delta V$	$\Delta$(V-I)
	2440000+		(mag)	(mag)	(mag)	(mag)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
030456	9349.6220	7	8.064	.017	9.801	.022	7	.41	.02	.46	.04	1.737	.05
030593	9348.6066	6	7.262	.017	9.039	.017	6	.15	.02	.39	.02	1.778	.25
030840	9349.6093	7	6.033	.028	7.448	.083	0	-	-	-	-	1.415	-
030925	9347.5830	6	7.038	.017	8.597	.019	6	.07	.02	.04	.03	1.559	-.02
031042	8940.8325	11	8.969	.054	10.402	.054	11	.62	.07	.87	.07	1.433	.25
031126	9345.6288	9	10.743	.020	12.678	.020	9	1.79	.03	2.46	.03	1.935	.67
031539	9346.6124	16	9.335	.020	11.931	.020	17	1.03	.03	.73	.03	2.596	-.30
031634	9345.6382	9	9.679	.020	12.772	.024	9	1.94	.03	.98	.04	3.093	-.96
031634	9345.6382	9	9.695	.020	12.526	.029	9	1.80	.03	2.89	.04	2.831	1.09
031833	8941.8389	11	11.598	.017	13.039	.018	0	-	-	-	-	1.441	-
032069	9347.5969	9	7.075	.017	9.183	.025	8	-.03	.02	.20	.04	2.108	.23
032111	9348.6281	11	8.021	.017	11.108	.056	11	.51	.02	1.53	.07	3.087	1.02
033177	8939.8370	10	9.569	.024	10.123	.024	10	.03	.03	.01	.03	.554	-.02
033487	9349.6266	4	9.716	.019	9.987	.021	3	.55	.03	.48	.03	.271	-.07
033499	9346.6570	4	10.649	.022	13.564	.027	0	-	-	-	-	2.915	-
033770	9348.6349	14	7.432	.017	10.032	.018	15	-.09	.02	.46	.03	2.600	.55
033900	9346.6613	4	8.811	.020	9.174	.020	4	-.04	.03	.09	.03	.362	.13
033969	9349.6428	14	8.223	.017	10.709	.022	13	.06	.02	.55	.03	2.486	.49
034000	9349.6484	4	5.814	.020	6.801	.030	4	-.31	.03	.12	.03	.987	.42
034386	9347.6434	11	8.065	.017	10.717	.023	11	-.13	.02	.60	.04	2.652	.73
034586	9349.6618	3	8.704	.019	9.540	.022	4	.33	.03	.45	.03	.836	.12
034817	9347.6500	11	6.075	.017	8.155	.027	11	-.14	.02	.11	.04	2.080	.25
034898	9348.6523	7	7.873	.017	10.132	.017	7	-.05	.02	.29	.02	2.259	.34
034919	9347.6839	14	7.456	.017	11.343	.084	1	.01	.02	.82	.09	3.888	.80
035207	8940.8604	5	8.174	.052	10.006	.052	5	.15	.07	.47	.07	1.833	.33
035391	9347.6614	3	7.641	.017	7.873	.017	1	-.12	.02	-.14	.02	.232	-.02
035439	9347.6665	11	7.926	.017	10.689	.020	10	.49	.02	.87	.03	2.763	.38
035539	9348.6767	1	8.304	.017	9.080	.018	3	-.02	.02	-.05	.03	.777	-.03
035924	9346.6712	4	10.361	.020	10.379	.020	4	.78	.03	.79	.03	.017	.01
036013	9349.6694	11	9.572	.017	11.274	.020	11	-.14	.02	.20	.03	1.702	.34
036108	9346.6759	4	10.161	.024	11.355	.043	4	.65	.03	3.35	.05	1.194	2.70
036442	9348.6946	5	8.811	.018	10.991	.044	11	1.19	.03	.38	.10	2.180	-.81
038137	9346.6847	4	8.977	.020	10.121	.021	4	-.67	.03	-.29	.03	1.144	.38
039290	9346.6884	4	8.203	.020	9.324	.020	4	-.17	.03	.17	.03	1.121	.35
039498	9346.7030	7	9.323	.021	10.688	.034	7	.74	.03	.84	.07	1.365	.10
043422	9345.7281	3	9.669	.020	9.959	.020	6	1.58	.03	1.72	.03	.290	.14
043539	9348.7327	4	7.400	.018	9.164	.025	1	.04	.02	.31	.03	1.764	.27
043708	9345.7341	3	12.019	.020	15.948	.051	3	2.61	.03	3.48	.06	3.929	.87
043920	9348.7458	3	7.262	.017	7.387	.017	3	.42	.02	.42	.02	.125	.00
044429	9349.7512	3	8.503	.017	11.550	.018	4	.27	.02	.68	.02	3.046	.41
044776	9347.7340	14	7.867	.017	10.735	.017	13	.09	.02	.70	.02	2.869	.62
045582	9349.7403	3	9.249	.017	9.689	.017	3	.68	.02	.73	.02	.440	.06
077311	8851.5231	11	8.743	.020	11.805	.020	10	.10	.03	.58	.03	3.062	.48
078163	8851.5294	2	9.058	.020	10.320	.021	3	.71	.03	.90	.03	1.262	.19
079960	8851.5429	3	8.392	.020	9.397	.020	3	.07	.03	.37	.03	1.005	.29
080540	8851.5703	3	10.508	.020	10.736	.020	3	1.27	.03	1.24	.03	.228	-.03
083530	8850.5728	16	9.886	.020	12.452	.020	17	.55	.03	.67	.03	2.567	.12
085306	8849.5645	5	9.409	.025	11.565	.025	6	1.05	.04	.45	.04	2.155	-.60
085685	8849.5822	12	8.962	.025	10.073	.025	0	-	-	-	-	1.111	-
086632	8852.5419	3	9.684	.020	9.918	.020	3	.66	.03	.69	.03	.234	.03

 

Table 4: continued.

Identifier	Jul. Dat.	nV	$V_{\rm A}$	$\sigma_{V_{\rm A}}$	$V_{\rm B}$	$\sigma_{V_{\rm B}}$	nI	$(V-I)_{\rm A}$	$\sigma_{(V-I)_{\rm A}}$	$(V-I)_{\rm B}$	$\sigma_{(V-I)_{\rm B}}$	$\Delta V$	$\Delta$(V-I)
	2440000+		(mag)	(mag)	(mag)	(mag)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
087176	8851.6328	14	10.288	.020	12.570	.020	15	.75	.03	1.24	.03	2.282	.49
087535	8852.5554	3	9.394	.020	10.374	.020	3	.60	.03	.70	.03	.980	.11
087718	8851.6572	13	8.861	.020	11.452	.020	13	1.20	.03	.73	.03	2.591	-.47
087914	8852.5610	3	8.677	.020	9.280	.020	3	.85	.03	1.12	.03	.602	.27
088203	8852.5766	6	9.209	.020	11.339	.020	6	1.11	.03	.65	.03	2.130	-.45
090189	8852.6030	3	10.215	.020	10.367	.020	0	-	-	-	-	.152	-
090574	8851.6638	3	8.130	.020	8.222	.020	6	.66	.03	.67	.03	.092	.01
090787	8852.6200	3	9.873	.020	10.214	.020	5	.48	.03	.55	.03	.342	.08
091380	8851.6781	9	8.174	.020	10.360	.020	3	.00	.04	.03	.04	2.183	.03
091754	8852.6250	4	8.536	.020	9.728	.020	3	.55	.03	.68	.03	1.193	.14
092415	8850.6263	12	8.283	.020	12.070	.020	13	.52	.03	.73	.03	3.787	.21
092560	8849.6048	14	9.421	.025	11.863	.025	14	.63	.04	.67	.04	2.441	.04
093069	8852.6397	3	9.383	.020	9.911	.020	3	1.87	.03	2.07	.03	.528	.19
093521	8849.6164	4	11.183	.025	12.465	.025	4	1.36	.04	1.82	.04	1.283	.46
093970	8852.7062	3	10.341	.020	10.478	.020	3	.70	.03	.71	.03	.137	.01
094307	8849.6550	11	9.776	.035	13.027	.035	14	.70	.04	1.29	.04	3.252	.58
095097	8850.6447	2	9.961	.020	11.336	.020	2	.40	.03	.62	.03	1.375	.21
095493	8852.6464	3	10.602	.020	10.629	.020	3	.49	.03	.50	.03	.027	.01
096667	8848.6367	4	7.426	.025	7.490	.025	5	.33	.04	.35	.04	.064	.02
096915	8850.6513	3	9.458	.020	10.398	.020	3	.83	.03	1.25	.03	.940	.42
097301	8848.6694	12	7.696	.025	10.543	.026	4	.38	.04	.84	.04	2.847	.47
097570	8850.6669	7	8.349	.020	10.791	.020	7	.07	.03	.44	.03	2.442	.38
097593a	8849.6674	3	6.958	.025	11.474	.026	3	1.03	.04	.79	.04	4.516	-.24
097593a	8852.6607	1	6.932	.021	11.526	.021	0	-	-	-	-	4.594	-
100182	8851.6862	13	10.152	.020	12.415	.020	14	.71	.03	1.32	.03	2.263	.61
101317	8852.7115	3	10.699	.020	10.756	.020	3	1.65	.03	1.67	.03	.057	.02
101653	8849.6992	4	8.999	.025	12.593	.026	20	1.17	.04	1.08	.04	3.594	-.09
102467	8852.7274	3	10.865	.020	13.726	.020	3	.66	.03	.69	.03	2.861	.03
102532a	8848.7300	3	4.264	.025	5.157	.025	4	1.04	.04	.60	.04	.893	-.44
103438	8852.7324	4	8.495	.020	8.983	.020	3	.59	.04	.86	.04	.488	.28
103475	8850.6935	4	9.640	.020	9.929	.020	1	.39	.03	.11	.03	.290	-.29
104370	8852.7473	3	10.264	.020	10.640	.020	3	.76	.03	.84	.03	.377	.08
104582	8850.7053	3	9.455	.020	10.930	.020	3	.43	.03	.50	.03	1.475	.06
105692	8851.7347	16	9.306	.020	11.165	.020	16	.73	.03	.81	.03	1.859	.08
105842	8851.7438	13	8.944	.020	11.817	.020	13	-.04	.03	.56	.03	2.873	.60
106411	8850.7115	4	10.135	.020	10.979	.020	4	.57	.03	.77	.03	.844	.20
106602	8850.7283	6	10.118	.020	11.327	.020	7	.87	.03	1.33	.03	1.209	.46
107206	8852.7558	3	10.660	.020	11.054	.020	3	.55	.03	.60	.03	.394	.05
107658	8850.7347	5	9.415	.020	10.915	.020	6	.65	.03	1.12	.03	1.500	.47
108801	8851.7629	8	8.215	.020	9.975	.020	8	.35	.03	.57	.03	1.760	.21
109183	8851.7685	4	8.957	.020	10.183	.020	3	.71	.03	.94	.03	1.226	.23
109840	8851.7854	6	8.634	.020	10.622	.028	6	.26	.03	.67	.04	1.989	.41
110654	8939.5889	4	9.692	.022	11.248	.022	4	.14	.04	.39	.04	1.556	.25
111231	8941.5226	4	9.490	.015	11.246	.015	4	.60	.02	.88	.02	1.757	.29
111687	8852.7945	10	9.630	.020	12.273	.020	10	.63	.03	.58	.03	2.643	-.05
113386	9670.5303	9	7.679	.025	9.286	.025	10	.75	.04	.81	.04	1.607	.06
113537	8850.8008	6	8.232	.020	9.506	.020	6	.57	.03	.68	.03	1.274	.11
114167	8848.8258	3	6.297	.025	7.100	.025	5	.55	.04	.61	.04	.803	.06
114378a	8850.7841	3	6.543	.020	10.275	.021	1	.60	.03	1.56	.03	3.731	.97
114857	8852.8049	14	8.791	.020	11.541	.021	14	.88	.03	.65	.03	2.750	-.24

 

Table 4: continued.

Identifier	Jul. Dat.	nV	$V_{\rm A}$	$\sigma_{V_{\rm A}}$	$V_{\rm B}$	$\sigma_{V_{\rm B}}$	nI	$(V-I)_{\rm A}$	$\sigma_{(V-I)_{\rm A}}$	$(V-I)_{\rm B}$	$\sigma_{(V-I)_{\rm B}}$	$\Delta V$	$\Delta$(V-I)
	2440000+		(mag)	(mag)	(mag)	(mag)		(mag)	(mag)	(mag)	(mag)	(mag)	(mag)
115863	8852.8251	6	8.872	.020	10.610	.021	3	.31	.03	.41	.03	1.738	.10
116068	8850.8134	5	9.311	.020	10.909	.020	6	.51	.03	.60	.03	1.599	.09
116737	8848.8578	4	6.628	.039	7.405	.039	4	.30	.05	.40	.05	.777	.10
116748	8852.8310	4	8.503	.020	9.710	.020	4	.77	.03	1.10	.03	1.206	.34
117081	9668.5409	6	9.697	.021	9.789	.021	4	.64	.03	.66	.03	.092	.02
117269	8941.5436	5	9.410	.016	9.468	.016	6	.47	.02	.47	.02	.057	-.01
117598	8941.5616	14	8.873	.016	11.375	.017	15	.60	.02	.82	.02	2.502	.23
ADS6223	9345.6941	6	9.011	.017	10.387	.017	9	.14	.02	1.90	.03	1.376	1.76
042581a	9345.6621	3	7.738	.020	9.910	.025	0	-	-	-	-	2.172	-
-1504995a	8850.5992	3	9.475	.020	9.506	.020	0	-	-	-	-	.031	-
032144a	9347.5462	3	6.256	.017	8.367	.017	3	.32	.02	.71	.03	2.111	.39
032144a	9348.5582	6	6.245	.017	8.356	.017	7	.32	.02	.66	.02	2.111	.35
005843a	8851.9178	3	7.536	.020	11.881	.026	0	-	-	-	-	4.345	-
005843a	8852.8897	3	7.534	.020	11.870	.022	0	-	-	-	-	4.336	-
005843a	9345.4642	3	7.027	.020	11.259	.022	0	-	-	-	-	4.231	-
005843a	9347.4026	3	7.623	.017	11.886	.017	3	2.15	.02	.70	.03	4.263	-1.45
005843a	9349.4065	3	7.621	.017	11.891	.018	3	2.17	.02	.76	.03	4.270	-1.41
000248a	9346.4267	5	8.467	.020	9.564	.020	3	.20	.03	.75	.03	1.097	.55
+1303203a	8848.5108	3	9.099	.032	9.595	.033	2	.75	.04	.84	.04	.496	.08
+1303203a	8849.4945	3	9.071	.025	9.564	.025	3	.73	.04	.80	.04	.493	.07
+1303203a	8850.5132	6	9.072	.020	9.567	.020	9	.75	.03	.83	.03	.496	.08
+1303203a	8851.4831	5	9.101	.020	9.593	.020	3	.75	.03	.83	.03	.491	.08
+1303203a	8852.4996	3	9.092	.020	9.574	.020	0	-	-	-	-	.482	-

Figure 2: Distribution of differences in relative position, d, between filters V and i for the 225 systems discussed in the text. Black fields represent the 15 systems with $\rho < 3\hbox {$^{\prime \prime }$ }$ and $\Delta i > 2$  mag.